Ivan Logashenko for Mu2e Collaboration Workshop on e+e- collisions from Phi to Psi, Sep.19-22, 2011...

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Ivan Logashenkofor Mu2e Collaboration

Workshop on e+e- collisions from Phi to Psi, Sep.19-22, 2011Novosibirsk, Russia

Search for cLFVWe had several talks on cLFV already – MEG, COMET, BELLE,…

Why is it interesting?Charged Lepton Flavour Violation in SM is extremely small. Any detectable signal is a sign of New Physics.

Why muons?Copiusly produced

We are trying to measure

Standard Model predicts extremely small value:

( , ) ( , )

( , ) ( , 1)e

A Z e A Z

A Z AR

Z

2* 541

22W,3

3) 10

32Br( k

k ekk

me U

MU

Novosibirsk, 20112 e+e- collisions from Phi to Psi

History of Mu2eThe current best limit was obtained at SINDRUM II experiment (90’s-2000)

Mu2e is the successor of two earlier proposals:

• MELC at Moscow, early 90’s

The main ideas of the experimental design were proposed

• MECO at Brookhaven, early 2000’s

Part of RSVP program, along with KOPIO, search for K->pinunu

At lof of design work and R&D were performed before the program was terminated

Mu2e goal:

137 10e

Au AuR

Au

e

capture

17 (90% c.l.6 10 )e

e

captu

Al AlR

Al re

Novosibirsk, 20113 e+e- collisions from Phi to Psi

Mu2e vs MEG

2( 1)CLFV R L

mL e F

k

2(1 ) L L L L L Le u u d dk

k

“Model-independent” lagrangian:

<< 1magnetic moment

type → e rate ~300X

N → eN rate >> 1

four-fermion interation almost no

contribution to → e

μ → eγ decay and μN → eN conversion are complementary

Mu2e

Mu2e @ProjectX

MEG

SINDRUM IIMEGA

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MEG 2011

Overview of the technique

Stop muons in aluminum

Muons quickly get to 1S orbit

Lifetime of muonic atom is 864 ns

Look for 105 MeV electron

- decay (40%)ee

- capture (60%)XAl

- conversionAl e Al

Hydrogen-like atomBohr radius ≈20 fmNucleus radius ≈4 fm

Most of the background is well below this energy

Use X-rays to monitor number of muons

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Background: Muon decay-in-orbit (DIO)

Free muon In-orbit

Long tail!

For decay-in-orbit , the maximum energy of electron is equal to the energy of conversion electron (≈105 MeV).

The high-energy tail

Need good energy resolution to beat this background!

5

convE E

eeAl Al

Novosibirsk, 20116 e+e- collisions from Phi to Psi

Background: Radiative muon capture (RMC)

This background is mostly low energy, but:

Radiative Muon Capture:• with small BR≈10-5, γ’s from muon captures can have high energy up to

• source of high energy electrons, comparable with DIO at the tail: γ can convert in target to e+e- pair, and electron can get almost all energy

• With good energy resolution and proper choice of target (MZ-1>MZ) this source of background is under control

Al(27,13) Mg(27,12) 1.5 0.1 2n p

Muon capture is the source of many background particles:

2.5 MeV (for Al)N convmm E

Novosibirsk, 20117 e+e- collisions from Phi to Psi

Background: Radiative pion capture (RPC)Muon are produced from pion decays, therefore there are pions in the muon beam.

Radiative Pion Capture:• pions stop at the target and promptly annihilate on the nucleus

• with BR~10-2, γ is produced with energy up to 137 MeV (for Al)

• source of high energy electrons: γ can convert in target to e+e- pair, and electron can enough energy to mimic conversion electron

• This is prompt background, it quickly dies away. Solution: pulsed beam.

(27,13) (27,12)Al Mg

Time distribution of stopped pions in the target

Novosibirsk, 20118 e+e- collisions from Phi to Psi

Overview of the design

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Production Solenoid 4 m longTransport Solenoid 13 m longDetector Solenoid 12 m long

Historical perspective: MELC proposal (1992)

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Production Solenoid

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Extinction

To avoid prompt background, we use pulsed beamThe signal is extremely rare

Need extinction factor 10-10!…and it has to be measured

Use combination of techniques to achieve this factor

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Accelerator

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Mu2e vs NOvA vs g-2

Mu2e can operate concurrently with FNAL neutrino experiments (NOvA)

we use 6 out of 18 Booster batches, which NOvA can’t use during Main Injector cycle

G-2 and Mu2e use the same beam, but in a different mannercannot run concurrently, but there is effort to make it possible to switch between the experiments

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Muon Beam Line

•Negative gradient

magnetic mirrow

no trapped particles

•Uniform field in tracker region

good resolution

•Torroidal field in the transport solenoid

separation/

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Transport Solenoid

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Stopping target

e

17 Al disks, 200 mkm thicknessWhy Aluminum? Perfect for this experiment

•higher Z: larger conversion ratedifferent contributions to the rate

•lower Z: larger lifetimehigher conversion energy

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T-tracker

18 stations x 12 panels x 2x50 straws =21600 straws

5 mm dia. Mylar straws, 15 μm walls, 20 μm Au-plated W wire

200 μm position resolutionNovosibirsk, 201118 e+e- collisions from Phi to Psi

Measuring the momentum

Low energy e- pass undetected

For high energy e- we detect several points on the helix

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CalorimeterLocated downstream of tracker

Main purpose: to provide trigger (1 kHz for E>80 MeV)Provides redundant position, timing and energy data

Possible design:2112 LYSO crystals, 3x3x13 cm3 arranged in 4 vanes. Density 7.3g/cm3, Moliere radius 2.07 cm, Rad. Length 1.14 cm, decay time 40 ns. Light yield relative to NaI 85%.

Two APDs per crystalNovosibirsk, 201120 e+e- collisions from Phi to Psi

Cosmic Ray Shield

Cosmic rays can generate high energy

electrons

Need high suppression factor – a lot of cosmic ray events over 2 year

running period

Combination of passive (magnetized

iron + dirt) and active (scintillation counters) shielding

99.99% coverage Novosibirsk, 201121 e+e- collisions from Phi to Psi

Expected sensitivity

Proton flux 1.8x1013 p/s

Running time 2x107 s

Total protons 3.6x1020 p

Stopped μ per proton 0.0025

μ capture probability 0.61

Time window 0.49

Trigger efficiency 0.80

Selection efficiency 0.19

Sensitivity (90% CL) 6x10-17

Events for Rμe=10-16 4

Estimated background 0.18

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What we expect to see

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Project schedule

e+e- collisions from Phi to Psi Novosibirsk, 201124

July 2005RSVP @BNL cancelled for financial reasons not related to MECO

October 2007

Mu2e LOI submitted to Fermilab

Fall 2008Proposal submitted to Fermilab and receives Stage I approval

November 2009

CD0 status granted

2010-2011 R&D and design, preparation of CDR2012 CD1

~2013 CD2, Start of Solenoid Construction~2018-2020 Start of data taking

Project X

There is proposal to replace FNAL’s Booster with new 8 GeV high-intensity linear accelerator, based on ILC technologies – “Project X”

Project X would feed neutrino and rare decay/high precision experiments

Potential to upgrade Mu2e by factor x100!• set much stronger limits (if there is no signal)

• or use different target materials to study nature of new physics (if there is signal)

Serious upgrade of the detector is required

Novosibirsk, 201125 e+e- collisions from Phi to Psi

ConclusionIn May 2008 P5 (US Particle Physics Project Prioritization Panel) Report stated:

“recommends pursuing the muon-to-electron conversion experiment under all budget scenarios considered by the panel.”

Why?• Mu2e experiment will allow to improve the current limit by 4 orders of magnitude

• if signal is found, it will be an undeniable proof of the New Physics and it will provide data, complementary to LHC

• if no signal is found, it will set constrains much stronger than LHC (up to 1000 TeV mass scale)

• with better muon source and other upgrades, the limits can be improved by another 2 orders of magnitude

Novosibirsk, 201126 e+e- collisions from Phi to Psi